SDO HMI 2014-08-03 09:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.33 | 0.00 | 8.76 | 15.31 | 258.43 | 19.28 | 301.02 | 0.3744 | 459.8 | 347.3 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.73 | 17.14 | 268.69 | 29.54 | 293.73 | 0.5167 | -597.0 | -532.3 | |
| 0.00 | 1.81 | 0.00 | 1.04 | 15.87 | 268.00 | 28.85 | 291.71 | 0.5016 | -533.0 | -476.8 | |
| 0.00 | 1.00 | 0.00 | 0.57 | 15.89 | 267.57 | 28.42 | 291.98 | 0.4956 | -784.0 | -633.6 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 9.28 | 260.73 | 21.58 | 280.21 | 0.3704 | 717.0 | 602.1 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 11.75 | 260.02 | 20.86 | 287.19 | 0.3666 | 853.0 | 659.6 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 9.51 | 258.57 | 19.42 | 281.73 | 0.3364 | 885.0 | 727.1 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 14.68 | 256.88 | 17.73 | 298.03 | 0.3352 | 849.0 | 647.7 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 17.62 | 257.06 | 17.91 | 305.27 | 0.3605 | 840.0 | 660.3 | |
| 0.00 | 0.91 | 0.00 | 0.52 | 30.82 | 259.13 | 19.98 | 325.45 | 0.5195 | 697.0 | 557.9 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 12.23 | 255.85 | 16.69 | 292.07 | 0.3042 | 874.0 | 723.6 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 12.11 | 255.48 | 16.33 | 292.11 | 0.2980 | 856.0 | 620.6 | |
| 0.00 | 2.81 | 0.00 | 1.42 | 17.18 | 243.71 | 4.55 | 338.77 | 0.2104 | 861.0 | 716.6 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |